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SLAU2-MHD for Low Mach Magnetohydrodynamics (MHD) Simulations [PDF]
AIAA AVIATION 2021 FORUM, 2021 Takashi Minoshima +2 more
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2007
In this chapter we will explain the basic MHD equations which are needed to understand solar active phenomena such as spots, prominences, flares etc.
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In this chapter we will explain the basic MHD equations which are needed to understand solar active phenomena such as spots, prominences, flares etc.
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MHD stagnation point flow of viscoelastic nanofluid with non-linear radiation effects
, 2016M. Farooq +5 more
semanticscholar +1 more source
Global well-posedness for the 2D MHD equations without magnetic diffusion in a strip domain
, 2016Xiaoxia Ren, Zhaoyin Xiang, Zhifei Zhang
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Entropy generation in steady MHD flow due to a rotating porous disk in a nanofluid
, 2013Mohammad Mehdi Rashidi +2 more
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Magnetohydrodynamics of the Sun: The Basic Equations of Magnetohydrodynamics (MHD)
, 2014E. Priest
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Chapter 3: MHD stability, operational limits and disruptions
, 2007T. Hender +57 more
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